Many scientists believe the Earth was dry when it first formed, and that the building blocks for life on our planet — carbon, nitrogen and water — appeared only later […]
astrochemistry
Rotational Spectroscopy, Tentative Interstellar Detection, and Chemical Modelling of N-methylformamide
N-methylformamide, CH3NHCHO, may be an important molecule for interstellar pre-biotic chemistry because it contains a peptide bond. The rotational spectrum of the most stable trans conformer of CH3NHCHO is complicated […]
First Detection of Methyl Isocyanate (CH3NCO) in a Solar-type Protostar
We report the first detection of the prebiotic complex organic molecule CH3NCO in a solar-type protostar, IRAS16293-2422 B. This species is one of the most abundant complex organic molecule detected […]
The Elements of Life Mapped Across the Milky Way by SDSS/APOGEE
To say “we are stardust” may be a cliché, but it’s an undeniable fact that most of the essential elements of life are made in stars. At today’s American Astronomical […]
Glycolaldehyde In Perseus Young Solar Analogs
Aims: In this paper we focus on the occurrence of glycolaldehyde (HCOCH2OH) in young solar analogs by performing the first homogeneous and unbiased study of this molecule in the Class […]
Expanding the Catalog: Considering the Importance of Carbon, Magnesium, and Neon in the Evolution of Stars and Habitable Zones
Building on previous work, we have expanded our catalog of evolutionary models for stars with variable composition; here we present models for stars of mass 0.5 – 1.2 Msol, at […]
Search for Interstellar Monohydric Thiols
It has been pointed out by various astronomers that very interesting relationship exists between interstellar alcohols and the corresponding thiols (sulfur analogue of alcohols) as far as the spectroscopic properties […]
Carbon Abundances in Stars With and Without Planets Using The CH Band
Context. Carbon, oxygen and nitrogen (CNO) are key elements in stellar formation and evolution, and their abundances should also have a significant impact on planetary formation and evolution. Aims. We […]
First detections of ethylene oxide, acetone and propanal toward the low-mass protostar IRAS 16293-2422
One of the open questions in astrochemistry is how complex organic and prebiotic molecules are formed. Aims. Our aim is to start the process of compiling an inventory of oxygen-bearing […]
Meteorites and the RNA World: A Thermodynamic Model of Nucleobase Synthesis within Planetesimals
The possible meteorite parent body origin of Earth’s pregenetic nucleobases is substantiated by the guanine (G), adenine (A) and uracil (U) measured in various meteorites. Cytosine (C) and thymine (T) […]
